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14 protocols using sp2300

1

Time-Resolved Emissive States Measurement

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For the detection of the time-resolved emissive states, the home-built transient grating PL technique (62 (link)) was used. The setup was pumped with a femtosecond (<150 fs) Ytterbium fiber laser (Tangerine SP, Amplitude Systemes; operating at 58 kHz, centered at 1,030 nm). The output of the laser was split into the pump and gate parts. The pump was frequency tripled to 343 nm using a home-built setup. The sample’s PL signal was collected and refocused onto a gate medium (1-mm fused silica crystal). The gate part of the beam was split using a 50/50 beam splitter to generate two gate beams. These beams were then focused onto a gate medium at a crossing angle of 8° and overlapped with the PL signal using boxcar geometry (63 ). The spatial and temporal overlap of the gate beams inside a gate medium created a laser-induced transient grating, acting like an optical shutter to resolve the broadband PL signals. Two achromatic lenses collimated and focused the gated signals onto the spectrometer entrance (Princeton Instruments SP 2300), and the gated PL spectra were measured by an intensified charge-coupled device (CCD) camera (Princeton Instruments, PIMAX3). The time delay between the pump and the gate beams was controlled via a motorized delay line, and 120,000 shots at each gate time delay were accumulated.
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2

Optical Characterization of Small Samples

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The optical measurements were performed using a homemade spectroscopy system designed to characterize samples with small sizes. For transmission spectral measurement, white light from tungsten halogen source (HL-2000, Ocean Optics) or supercontinuum light sources (SC400-4, Fianium) was collimated and confined to proper beam size, which was then weakly focused onto the sample by a near-infrared (NIR) objective lens [×10, 0.25 numerical aperture (NA); Olympus]. The transmitted signals were collected using another NIR objective lens (×100, NA 0.9; Olympus) and delivered to a spectrometer (SP-2300, Princeton Instruments) equipped with a liquid nitrogen–cooled charge-coupled device (CCD) detector (PyLoN-IR). An NIR CCD camera (XS-4406, Xenics) was set within the switching optical path for imaging. For measurement of CD, a linear polarizer (650 to 2000 nm; Thorlabs) and a quarter-wave plate (1100 to 2000 nm; Thorlabs) were inserted into the input optical path at specific orientations. Therefore, the spectra in this work were mainly focused on wavelength range from 1100 to 2000 nm. Linear polarization rotation experiments were conducted by varying the detection polarization (linear polarizer, 650 to 2000 nm; Thorlabs) at every 15° under linearly polarized incidence.
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3

Femtosecond SFG Spectroscopy with UV Illumination

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The SFG experiments were carried out with a femtosecond broadband laser system. Briefly, a Ti:sapphire amplifier (Spitfire ACE, Spectra Physics) produces ~7 W of 800-nm, 35-fs pulses at a 2-kHz repetition rate. Forty percent of the 800-nm beam passed through a beam splitter to pump an optical parameter amplifier followed by a difference frequency generation stage (TOPAS-C, Spectra Physics). The rest was reflected from a Bragg filter (N013-14-A2, OptiGrate) to generate a narrow band beam of ~0.5-nm bandwidth. The broadband IR and narrowband 800-nm pulses overlapped at the sample surface with incident angles of 57° and 45°, respectively. The SF signal was collected along the reflected direction with a spectrograph (Acton SP2300) and a liquid nitrogen–cooled charge-coupled device camera (Princeton Instruments PyLoN 1340×100).
The UV illumination was carried out in vacuum at a base pressure of 10−7 torr to exclude ambient oxygen. The UV lamp illuminated the sample at a power density of about 0.9 mW/cm2 with a wavelength centered at 365 nm (see fig. S3). SF spectra reported in the main text were taken with the SSP polarization combination at 295 K after 30 min of UV illumination.
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4

Raman Spectroscopy of Macrophage Cells

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Raman spectroscopy (Horiba Jobin Yvon (Paris, France) of macrophage cells was performed using a 532 nm laser (Sapphire SF-532; Coherent, Santa Clara, CA) excitation and NA/1.35 oil-immersion objective lens focusing the laser beam on the sample. The back scattered Raman signal was passed through the filters and focused on the slit of the spectrograph SP2300; Princeton Instruments, Acton, MA) with 1200 lines/mm grating of the signal light. The sample scaffold was deposited on a glass bottomed dish placed on the Raman x-y-z stage. All Raman spectrums were obtained at room temperature (23 °C) in the same environment with a laser power at 10mW in between 400 and 1800 cm-1 in 60 s. All measurements were recorded using WinSpec software and processed using Matlab (The MathWorks, Natick, MA) while preprocessed by the same method. All instrumental response and wavelength positions were calibrated. For Raman spectra, three different locations were selected for each group.
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5

High-Harmonic Generation in Graphene

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Based on femtosecond laser system (Light Conversion PHAROS), mid-infrared pulses are prepared using optical parametric amplifier (ORPHEUS) and difference frequency generator (LYRA). The output serves wavelength-tunable multi-cycle pulses with repetition rate of 100 kHz. The spectral linewidth of the pulse is 15.4 meV in full-width half-maximum and the pulse duration is estimated to be 120 fs assuming a Fourier-transform-limited pulse. To control its ellipticity, liquid crystal retarder (Thorlabs LCC1111-MIR) is employed, whose optical axis is oriented at an angle of 45° with respect to the laser polarization. Then, mid-infrared pulses are focused at roughly center of the graphene device by ZnSe focusing objectives with spot size of 150 μ m. Emitted HHG has been collected by 50X objective lens on transmission geometry, and its polarization is analyzed by half-wave plate mounted on motorized stage and fixed Glan-Taylor polarizer. The HHG spectra are recorded by an electron-multiplying charge-coupled device detector (ProEM, Princeton instruments) and grating spectrometer (SP-2300, Princeton instruments) at Materials Imaging & Analysis Center of POSTECH.
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6

Optical Imaging and Electrochemistry of AuNP on MoS2

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The optical imaging of a single AuNP on an MoS2 monolayer-covered gold film was measured by an inverted dark-field microscope (Eclipse Ti-U, Nikon), which was equipped with an oil-immersed dark-field condenser (NA = 1.20 to 1.43), a water-immersed objective lens (NA = 0.6, 40×, part number MRH08430), and a quartz tungsten halogen lamp (LV-LH50PC, Nikon) as the light source. The dark-field scattering spectrums of a single AuNP on MoS2 monolayer-covered gold film were captured by a grating spectrometer (Acton Spectra Pro SP-2300, Princeton Instruments) equipped with a liquid-nitrogen-cooled charge-coupled device (CCD). The extinction spectra of individual AuNPs on MoS2 monolayer surfaces were measured by a spectrometer (SP-2-300, Princeton Instruments) and an electron-multiplying charge-coupled device (EMCCD) camera (ProEM+, Princeton Instruments). The electrochemical measurements were carried out with three-electrode system by an Autolab (Autolab PGSTAT302N, Metrohm AG). The square step potential can be applied on the sample and the corresponding current of the entire electrode is recorded by the Autolab. The Ag/AgCl wire and Pt coil were used as the reference electrode and the counterelectrode, respectively. The MoS2 monolayer-covered gold film was the working electrode. The electrolyte is 0.1 M NaF aqueous solution.
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7

Optical Characterization of Nanowire Switches

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The optical measurements were performed on a home-built confocal microphotoluminescence system (fig. S17). A single wire was locally excited with a 351-nm laser beam (BeamLok 2065, Spectra-Physics) focused by an objective lens (50×; numerical aperture, 0.8; Nikon CFLU Plan). The emission of the wire was selectively collected from the tip using a confocal microscopy setup with a 1-μm pinhole. The light was subsequently coupled to a grating spectrometer (Acton SP2300) with a matched thermal electrically cooled charge-coupled device (ProEm: 1600 × 200B, Princeton Instruments).
For the measurements of electric field–induced asymmetric light propagation, an external electric field was applied with a commercial dc voltage supplier. The pulsed electric field was applied using a nanosecond signal generator, which supports tunable amplitude, frequency, and rise time (fig. S18). The optical signals were detected using a silicon photodetector and monitored using an oscilloscope to obtain the response time and switching frequency of the switch.
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8

Micro-spectroscopy Setup for Samples

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The employed micro-spectroscopy setup has been described elsewhere60 (link). Briefly, solid-state laser beams of 457.8 and 514.3 nm (Cobolt, Twist, and Fandango) were focused onto samples within a spot size of ~1 μm using a microscope objective (×40, NA = 0.60). The signals were collected using a CCD camera (Princeton Instruments, PyLon) with a spectrometer (Princeton Instruments, SP2300). All measurements were performed in the ambient conditions unless noted otherwise. The average power was maintained below 2 μW to avoid unwanted photoinduced degradation.
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9

Ultrafast Transient Absorption Spectroscopy

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For time-resolved femtosecond TA measurements, the fundamental beam produced by the Yb:KGW laser (Pharos, 1030 nm, 20 W, 100 kHz; Light Conversion Ltd.) was separated into several light beams and sent to a homebuilt microscopic ultrafast pump-probe spectrometer collinearly and then lastly combined and focused by a microscope to a spot size of 1 μm. For the pump beam, one of the seed beams was introduced into a commercial noncollinear optical parametric amplifier (2H-NOPA, Light Conversion Ltd.) and a second harmonic generation crystal beta-barium borate (BaB2O4) to generate the pump light with a certain wavelength centered at 470 nm. For the probe beam, another seed beam was focused onto an yttrium-aluminum-garnet crystal (8 mm thickness) to generate continuum white light as the probe light. The temporal delay time between the pump beam and the probe beam was controlled via a high-resolution motorized delay stage (M-ILS250HA, Newport). The pump and probe pulses overlapped spatially at the sample, and the transmitted probe light was collected by a spectrograph (SP2300, Princeton Instruments) coupled to a nitrogen-cooled detector (PyLon100B, Princeton Instruments). The transient transmission signal was calculated by contrasting and normalizing the transmitted probe spectra with and without a pump beam: ΔT/T = (TpumpTunpump)/Tunpump.
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10

Characterization of LED Optical Properties

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LEDs were characterized by probing samples on an inverted confocal microscope. Samples were imaged through the ITO/glass substrate using a ×50, NA = 0.70 objective. Electrical measurements were performed using a Keithley 2602A source measure unit. Electroluminescence images were collected with a thermoelectrically-cooled monochromatic camera (QImaging, EXi-AQA-R-F-M-14-C), under 5 min of integration time. The images were used to estimate the EL power per single LED as per the process outlined in Supplementary Note 6. Electroluminescence spectra were collected using a monochromator (Princeton Instruments, SP2300) and a thermoelectrically cooled CCD (Princeton Instruments, PIXIS 100).
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